The galaxy appears as a flattened elliptical or lenticular type, exhibiting a smooth, centrally concentrated light distribution. The core is a bright yellow, indicative of an older stellar population. Moving outward, the galaxy gradually fades into a less defined, bluer halo. This bluer component suggests the presence of some younger, star-forming regions. However, these regions do not dominate the overall color profile. The lack of distinct spiral arm structures, large dust lanes, or significant tidal features supports the impression of a relatively undisturbed, evolved system. There may be a minor asymmetry present which could be from a minor disturbance event in the past.
