The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a bright, compact core that gradually fades into an extended halo. The color is generally homogenous, displaying a predominantly blue-green hue throughout the main body, with slight hints of red near the core. There is no visible evidence of spiral arms, dust lanes, or recent major merger activity. The overall morphology suggests a relatively relaxed system, although subtle asymmetries in the outer regions cannot be entirely ruled out. The lack of prominent features implies that the galaxy is likely dominated by an older stellar population, with relatively low ongoing star formation. There is a possible minor tidal interaction.
