The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is centrally peaked, exhibiting a gradual decrease in intensity outwards from the core. The galaxy displays a yellow-orange hue, indicative of an older stellar population. There is very little evidence of spiral arm structure or dust lanes. The overall morphology suggests a lack of significant recent star formation activity. Slight asymmetry may be present, possibly indicating minor gravitational interaction, though no major disturbance is evident. The galaxy exhibits a roughly rounded shape.
