The galaxy presents as a relatively smooth and centrally concentrated light distribution. The overall shape appears to be generally elliptical, deviating slightly from perfect circularity but not exhibiting a highly elongated or cigar-like morphology. There is no obvious spiral arm structure or prominent disk.

The color profile suggests a redder, more luminous core, transitioning to bluer hues in the outer regions. This color gradient implies a stellar population that is generally older in the galactic center, with a potential increase in younger, star-forming regions in the periphery.

There is no clear indication of ongoing major mergers or significant tidal disturbances. However, subtle asymmetries or faint extensions might indicate minor interactions or past accretion events. Based on its morphology and color, this galaxy is likely an elliptical or lenticular galaxy at moderate redshift. Further spectroscopic analysis is required to determine its precise classification and star formation history.
