This galaxy appears as a relatively smooth, elliptical-like object, exhibiting a concentrated luminosity profile. There is evidence of a possible merging event or gravitational interaction with a secondary object. The light from the galaxy has a redshift corresponding to approximately z = 0.24, indicating significant distance. The object is fairly round in shape and has an effective radius of approximately 5 kpc. The color gradient suggests the presence of an older stellar population with lower ongoing star formation. A significant portion of the galaxy's classification indicates a morphology with a generally smooth appearance. However, closer inspection suggests an irregularity or extension on one side, possibly indicative of a minor tidal disturbance or early stage merger, which could be associated with the second concentrated luminous area. The mass is estimated to be quite high for this galaxy.
