The galaxy presents as a somewhat diffuse, elliptical morphology. There is a high degree of central concentration with a gradual decline in surface brightness outward. The color profile appears relatively uniform, with a slightly redder hue overall, suggesting a population dominated by older stars and a low rate of ongoing star formation. The overall structure is smooth and largely featureless, without obvious spiral arms, dust lanes, or signs of recent merger activity. A small perturbation may be occurring but difficult to identify. The object exhibits a round shape, and does not appear to be highly elongated or irregular. Based on these observed characteristics, this galaxy is likely an elliptical galaxy located at a redshift distance.
