The galaxy presents as a luminous, elliptical structure. A bright, concentrated central bulge dominates the visual profile, characterized by a yellowish hue indicative of an older stellar population. Moving outwards from the core, there appears to be a faint, diffuse halo. The galaxy lacks distinct spiral arm structures or prominent dust lanes, lending credence to its classification as an elliptical. The overall morphology suggests minimal ongoing star formation within the galaxy, with the light signature being dominated by older, redder stars. The galaxy exhibits a slight elongation, deviating subtly from a perfectly circular shape, though the axis ratio is relatively high, closer to a circular profile. There is no clear evidence of tidal disturbances or ongoing mergers within this galaxy.
