The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The color profile suggests a population of older stars, evident in the yellow-red hue. There are no visible spiral arms or prominent dust lanes. The morphology indicates a highly symmetric, round form, without significant tidal disturbances or signs of merging activity. The overall structure suggests a well-relaxed system, potentially a lenticular or elliptical galaxy at intermediate redshift. Star formation activity appears low based on the color profile, but the galaxy remains clearly visible within our observational limits.
