The galaxy presents a relatively smooth, elliptical morphology. The core exhibits a concentrated luminosity, transitioning to a more diffuse halo. The overall color profile suggests an older stellar population, with a redder hue dominating the central region. The galaxy appears elongated, possibly indicative of an E4-E6 classification on the Hubble sequence. There is no obvious dust lane or spiral arm structure visible, suggesting a lack of significant ongoing star formation. The galaxy's shape is likely close to being in-between rounded and cigar-shaped, leaning closer towards the cigar-shape. There is no evidence of any major merger or disturbance within the galaxy, only faint and subtle disturbances.
