The galaxy presents as a relatively smooth, elliptical-like morphology. Its color is primarily yellowish-white, concentrated towards the central region, suggesting an older stellar population dominates. The light distribution fades gradually from the core, with minimal evidence of distinct spiral arms or prominent dust lanes. There may be a faint disk surrounding the central bulge, oriented at a slight angle to our line of sight. No strong indications of recent or ongoing major merger activity are apparent, although there is a subtle irregularity that *could* be a minor disturbance. The galaxy exhibits a somewhat lenticular shape.
