The galaxy presents as an elliptical system, exhibiting a smooth, centrally concentrated luminosity profile. The object's overall shape appears somewhat flattened, transitioning from a more circular central bulge to a slightly elongated outer region. The color profile suggests a dominant population of older stars, with a yellowish-red hue indicating a relatively quiescent star formation rate. There is no evidence of prominent spiral arms or significant dust lanes. Faint, asymmetric extensions are seen but they do not show obvious signs of tidal interaction with other galaxies.
