The galaxy presents as a single, relatively smooth object with an elliptical morphology. The color profile suggests an older stellar population, concentrated toward the galaxy's core, and exhibiting redder hues. There is minimal evidence of active star formation within the observable region. The galaxy is generally round, with no significant disturbances or merging features visible. There appears to be a slight elongation along one axis, which indicates a potentially cigar-like shape. The overall appearance is consistent with a relatively evolved galaxy, possibly at a redshift of approximately 0.3, with a considerable stellar mass.
