The galaxy presents as a relatively smooth, elliptical object. It appears elongated, approximately cigar-shaped, suggesting a potential classification towards an E4-E6 elliptical galaxy, although a highly inclined disk galaxy cannot be ruled out without further spectral analysis. The central region exhibits high luminosity, indicating a concentrated stellar population or possibly an active galactic nucleus, though the data suggests otherwise. Faint, diffuse light extends from the central bulge. The color gradient displays a shift from bluer hues in the central areas to a more red-shifted tone in the outer regions, potentially indicating ongoing star formation localized near the core, or it could be indicative of varying stellar populations with age. There is a slight hint of a disturbance in the upper part of the galaxy, but it is likely to be natural elongation of the shape rather than a sign of a merger. The light profile seems fairly regular, suggesting a well-mixed stellar population across the galaxy.
