This galaxy presents as a relatively compact, early-type system, likely elliptical or lenticular in nature. The light distribution appears smooth and centrally concentrated with a high degree of roundness and a lack of spiral arm structure or prominent dust lanes. The color profile exhibits a moderate red hue, suggestive of an older stellar population with limited ongoing star formation. A slight asymmetry may be present in the outer regions, potentially indicating a past or ongoing minor interaction.
