This galaxy appears to be a relatively smooth, elliptical or lenticular type. The light distribution is centrally concentrated with a gradual decrease in intensity outwards. There is no obvious spiral arm structure or prominent dust lanes visible. The galaxy presents with an overall elliptical morphology, though with some deviation from a perfect ellipse. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue, characteristic of galaxies with lower star formation rates and a dominant population of evolved stars. There is a slight indication of possible minor disturbance in the form of a faint plume-like feature, suggesting past minor interactions.
