The galaxy presents a generally smooth morphology, with a concentrated central bulge. Its shape is elliptical, lacking distinct spiral arms or a pronounced disk structure. The light profile appears to gradually fade outwards from the core, suggesting a relatively uniform stellar population distribution in the outer regions. The galaxy exhibits a yellowish hue, indicative of an older stellar population. There's little evidence of significant dust lanes or active star formation regions. Overall, it gives the impression of a mature system. A very slight asymmetry in the outer regions could indicate a past minor merger event.
