The galaxy presents a generally smooth morphology, with a dominant spheroidal component. The core exhibits a yellowish hue, suggestive of an older stellar population. There is a slight extension to the upper right, which appears to have a redder color than the core, possibly caused by a population of dust-enshrouded red giant stars or recent star formation. There is little evidence of prominent spiral arm structures or significant dust lanes within the galaxy. The galaxy's overall shape is round, indicating a relatively relaxed dynamical state, though there are disturbances on the upper right side, suggestive of interactions with other objects. It may be undergoing a merger event with a smaller companion galaxy.
