The galaxy presents a somewhat elliptical morphology, although with noticeable irregularities in its outer structure. The central region exhibits a high surface brightness, appearing nearly uniform and unresolved. Moving outward, the luminosity decreases, but not in a completely smooth fashion. There are faint indications of a possible spiral arm structure or tidal debris extending outwards from the main body, primarily on the left side of the image. The color profile suggests a mixed stellar population, with a bluer component concentrated in the center and a redder component more prominent in the outer regions. There is a hint of minor disturbances on the left side that could indicate a past or ongoing interaction with a smaller object. 
