The galaxy presents as a somewhat compact object with a relatively smooth overall appearance, though with some noticeable substructure. The central region exhibits a higher concentration of luminosity, appearing nearly spherical. There is evidence of ongoing or recent interaction with at least one other galaxy, indicated by a more diffuse region of emission extending away from the main body. The color distribution suggests a moderately evolved stellar population overall, possibly with a population of younger stars in the disturbed regions. I observe that it is in a later stage of merging with another galaxy, or going through a tidal interaction. Star formation may be present but is likely subdued compared to more actively star-forming systems. The galaxy's profile suggests it could be elliptical, but the faint extended emission and indications of interaction make this uncertain. Further spectroscopic analysis is needed to determine the composition and dynamics of the system to confirm the nature of the features.
