The galaxy appears to be an elliptical morphology, exhibiting a generally smooth light distribution without prominent spiral arms or a well-defined disk. The galaxy has a moderate redshift, indicating a considerable distance. The color profile suggests a mix of stellar populations, with a slight central reddening possibly due to older stars and/or dust concentration, surrounded by bluer hues in the surrounding areas. The galaxy appears to be relatively undisturbed, without signs of major mergers or tidal interactions. The light profile is concentrated, with a round shape, suggesting a system that is supported by random motions. Overall, this galaxy likely hosts primarily an older stellar population with low ongoing star formation activity.