The galaxy presents as a relatively smooth, somewhat elliptical structure. It appears to be a large galaxy, with an estimated size of a few kiloparsecs across. There is no evident spiral structure or bar visible.

The color profile suggests a prominent bulge, indicated by a strong red/orange hue at the core, potentially indicative of an older stellar population. Surrounding the core is a less concentrated halo with green-yellow tones, suggestive of some ongoing star formation at the galaxy's edge. This may indicate younger stars and ionized gas in the outer regions. 

There are no signs of a major merger or significant tidal disturbances, suggesting it is not a galaxy currently undergoing a major interaction. There is no prominent dust lane or significant asymmetry apparent.
