The galaxy appears as a yellowish, moderately bright object, exhibiting a relatively smooth and elliptical morphology. It is characterized by a somewhat elongated, cigar-like shape, suggesting it may be an elliptical galaxy, possibly of type E4 or E5 on the Hubble sequence. The galaxy's light distribution is concentrated towards the center, with a gradual decrease in luminosity outwards. There are no discernible spiral arms, dust lanes, or significant features indicating ongoing major mergers or strong tidal disturbances. The overall color suggests an older stellar population dominating its composition. There is a possible slight asymmetry in its outer regions which could indicate minor gravitational interaction or a recent accretion event.
