The galaxy presents as a luminous, elliptical morphology. A bright central bulge dominates the structure, exhibiting a concentrated, yellowish hue, suggesting a significant population of older stars. The outer regions display a fainter, more diffuse glow with hints of blue, possibly indicating some level of ongoing star formation, although at a lower rate than the central bulge. The overall shape appears somewhat elongated, though with a generally smooth appearance, with a lack of prominent spiral arms or distinct features. There are some minor irregularities that might indicate a past or ongoing interaction with another galaxy, although no major merger or tidal disruption is obviously apparent.
