The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded with a slight elongation. The galaxy's core is luminous, displaying a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light fades into a blue tinge, indicating some presence of younger, hotter stars, perhaps due to moderate star formation. There is no evidence of significant spiral arm structure or tidal disturbances. The overall impression is that of a massive galaxy at a redshift of approximately 0.2, with a mass estimate suggesting it is a substantial system.
