The galaxy presents as a moderately luminous object with an elliptical morphology. It exhibits a centrally concentrated brightness profile, with the luminosity gradually decreasing towards the outer regions. There is an absence of any distinct spiral arm structures or prominent dust lanes, indicative of a relatively smooth stellar distribution. The galaxy appears yellowish-red in color, suggesting an older stellar population with a lower rate of ongoing star formation. Based on its relatively regular shape and lack of obvious tidal features, there is no strong evidence for recent or ongoing major merger activity. However, a slight asymmetry may indicate past minor interactions. The apparent size suggests that it is a moderately sized galaxy, based on its distance as measured by its redshift.
