The galaxy presents as a relatively smooth elliptical system, exhibiting a moderately elongated, cigar-shaped morphology. The central region is characterized by a concentrated bulge, exhibiting a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness, with a subtle transition towards a bluer color in the outer regions. There is minimal evidence of distinct spiral arms or prominent dust lanes. The overall smooth profile suggests a well-mixed stellar population. Subtle tidal disturbances or minor asymmetries are not readily apparent, indicating it's likely not undergoing any major merging events currently.
