The galaxy presents a smooth, elliptical morphology. The luminosity profile is centrally concentrated, with a bright core that gradually fades towards the outer regions. There is little to no evidence of spiral arm structure or significant dust lanes. The color is generally consistent with an older stellar population; redder hues dominate. The galaxy's shape is generally rounded, with a slight tendency toward being elongated rather than perfectly circular. There's no significant tidal disturbance, suggesting no recent major mergers. Overall, the galaxy is a well-defined elliptical with no prominent features indicative of active star formation or ongoing interactions.
