The galaxy presents as a smooth, elliptical-like structure, exhibiting a concentrated central bulge. Its color profile suggests an older stellar population, dominated by redder hues. There is no evidence of significant dust lanes or spiral arm structures. The galaxy appears to be relatively isolated with no clear signs of ongoing mergers or tidal disturbances. The object's morphology leans towards a spheroid shape, with minimal deviations from perfect roundness. A faint, diffuse halo appears to extend outward from the central region, gradually fading into the background. The overall appearance suggests a quiescent galaxy with low ongoing star formation.
