The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. The light distribution appears concentrated towards the core, suggesting an older stellar population dominates. The galaxy exhibits a yellowish-red hue, indicative of a relatively low star formation rate and a population of evolved stars. There is no apparent spiral arm structure or prominent dust lanes visible. Overall, the galaxy appears to be a passively evolving system, with a spheroid shape.
