The galaxy presents as a relatively smooth, though not perfectly symmetrical, structure. There is an indication of a central bulge, bright and yellowish, which suggests an older stellar population concentrated in the core. Fainter, bluish light surrounds the bulge, possibly indicating areas of more recent or ongoing star formation. However, this is not a dominant feature.

Overall, the galaxy has a noticeable reddish hue, suggesting that it is composed of older stars and potentially has some dust obscuration. There may be a faint disk, but no spiral arm structure is visible. The galaxy appears to be undergoing some gravitational disturbance, or perhaps a minor merger event, that is disrupting its smooth appearance.
