The galaxy presents as a relatively compact structure, exhibiting a somewhat elliptical morphology. The central region displays a pronounced luminosity, suggesting a high concentration of stellar populations or potentially an active galactic nucleus, although the image resolution does not allow for definitive determination of the latter. 

There is an apparent decrease in surface brightness from the core outwards, grading smoothly into the outer regions of the galaxy. A slight extension is observed along one axis, possibly indicative of a weak bar structure or tidal interactions with smaller companions. The overall color appears somewhat redder than average, consistent with an older stellar population and potentially lower levels of ongoing star formation. There appears to be little evidence of spiral arm structure or significant dust lanes within the galaxy. No significant merger activity is visible, though minor disturbances might be present. 
