The galaxy presents as a luminous, centrally concentrated object. The overall morphology appears largely spheroidal. There is a noticeable color gradient, shifting from a predominantly bluer hue in the outer regions to a slightly yellower, more concentrated core. The light distribution suggests a relatively smooth profile, with no obvious indications of spiral arms, rings, or a prominent disk structure. There is a slight elongation, deviating from a perfectly circular shape. No significant signs of recent or ongoing major mergers are evident. Subtle disturbances or minor interactions might be present, but are not distinctly visible at this resolution. The light profile suggests a galaxy dominated by an older stellar population, particularly within the central regions, with perhaps younger, bluer stars contributing to the overall light in the outskirts. Overall, this object is consistent with an early-type galaxy at moderate redshift.
