The galaxy presents as a somewhat amorphous, likely early-type system. There appears to be a high degree of central concentration, with a bright, unresolved core. Moving outward, the light profile fades gradually, showing a smooth appearance with little evidence of spiral arm structure or prominent dust lanes. The overall shape is elliptical, exhibiting moderate flattening but not distinctly disk-like. There is an observed color gradient, with the central region showing slightly bluer colors which may indicate recent or ongoing low level star formation. The outer regions appear redder, consistent with an older stellar population. A slight irregularity is visible on one side which could suggest a minor interaction or tidal disturbance. The overall luminosity suggests a reasonably massive galaxy.
