The galaxy presents an overall smooth appearance with a centrally concentrated luminosity profile, suggesting an elliptical morphology. There is little evidence of spiral arms or significant disk structure. The galaxy exhibits a moderate redshift, indicating that it is at a substantial distance from us. The color gradient appears subtle, with a possible trend toward redder hues in the central regions. There are no obvious signs of ongoing major mergers or tidal disturbances, although there is possibly some minor asymmetrical features. The overall shape appears somewhat round. Based on these features, it seems likely we are observing a relatively massive galaxy with a modest amount of star formation.
