The galaxy presents a relatively smooth morphology, appearing largely elliptical in shape with a high degree of central concentration. The light distribution suggests a lack of prominent spiral arm structures or strong tidal features, indicating a possibly evolved system. There is a slight but noticeable reddish-orange hue to the central regions, possibly indicative of an older stellar population. Fainter blue areas can be seen away from the center of the galaxy, possibly indicating areas of localized star formation. The overall extent of the galaxy appears moderate, neither exceptionally compact nor exceedingly large. The galaxy does not show any obvious signs of ongoing major mergers, although subtle disturbances or minor interactions cannot be ruled out.
