The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge with a notable lack of defined spiral arm structure. The color profile suggests a generally older stellar population, with a yellow-red hue indicative of evolved stars. The galaxy appears to be relatively isolated, showing no strong signs of tidal interaction or ongoing merger activity, though a minor disturbance cannot be ruled out due to the resolution limitations. Its shape is predominantly in between round and cigar shaped. The light distribution is fairly even, indicating a well-mixed stellar population and a lack of significant dust lanes or prominent star-forming regions. The overall appearance is consistent with an elliptical galaxy at a moderate redshift, characterized by a substantial stellar mass and relatively quiescent star formation.
