The galaxy presents as a moderately luminous object, with a generally smooth morphology. The shape appears to be elliptical, with a noticeable elongation along its major axis. A prominent central bulge is observed, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter, bluer light extends outwards from the bulge. The surrounding halo is diffuse, with an overall smooth appearance. There are no obvious signs of spiral arm structures or significant dust lanes. The overall color gradient suggests ongoing, but not overwhelming, star formation within the disk and bulge components. There appears to be a low chance of mergers or disturbances. The galaxy's orientation presents an intermediate inclination relative to our line of sight.
