The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, bright core, suggesting a high density of stars in its central region. The overall shape is generally round with a slight deviation towards an intermediate axis ratio. No prominent spiral arms or significant dust lanes are visible. Faint, diffuse light extends outwards from the core, gradually fading into the background. There is no strong indication of any recent or ongoing major merging events or significant tidal disturbances. The color appears to be somewhat redder, indicative of an older stellar population and relatively low ongoing star formation.
