The galaxy presents a distinct elliptical morphology, exhibiting a smooth, cigar-shaped structure. Its core displays a concentrated, bright yellowish-white luminosity, indicative of a substantial population of older stars and potentially a supermassive black hole actively accreting material at the center. The luminosity gradually diminishes towards the edges, transitioning into a more diffuse reddish halo. There appears to be minimal discernible dust obscuration or prominent spiral arm structures, which is consistent with a classification as an elliptical galaxy with a relatively low star formation rate. Minor asymmetric features or tidal disturbances are not visibly apparent, suggesting it is likely not undergoing a major merger event. The galaxy's overall color profile indicates a higher proportion of older stellar populations.
