The galaxy presents as a relatively compact object. Its morphology is largely smooth in appearance, exhibiting a centrally concentrated luminosity profile with no obvious spiral arm structure or distinct features. The galaxy's color is dominated by redder wavelengths, indicative of an older stellar population and potentially significant dust obscuration. There is a possible slight blue tint to the galaxy's halo, suggesting some ongoing, albeit subdued, star formation activity. The object is generally round. There appear to be no signs of ongoing major merger events or significant tidal disturbances, though there is a possible indication of some minor disturbance.
