This galaxy presents a morphology that is neither purely elliptical nor fully spiral, exhibiting characteristics of both. The central region displays a smooth, concentrated bulge with a yellow-white hue, indicating a significant population of older stars. A faint disk component surrounds the bulge, appearing somewhat irregular and exhibiting a slight blue tinge, possibly indicative of ongoing star formation.

There appears to be a smaller, irregular structure in close proximity to the galaxy, possibly undergoing a minor interaction. It exhibits a redder color, potentially signifying a population of older stars or significant dust obscuration. This neighboring structure could be a dwarf galaxy or a tidal feature resulting from a past interaction. 

The galaxy shows no prominent spiral arms and no obvious signs of significant recent merger activity, although some level of disturbance cannot be ruled out given the presence of the nearby irregular structure. Overall, the system appears to be in a relatively evolved state, with a moderate level of star formation activity.
