This galaxy appears to be an elongated, disk-shaped system. Its central region exhibits a bright, concentrated luminosity, possibly indicating a significant stellar population or an active galactic nucleus. The isophotes of this central region are smooth and regular. Extending outward from the core, the galaxy's luminosity decreases, showing a gradual fading into the surrounding background. There is a hint of a possible spiral structure, however, this is not clearly defined. The outer disk appears somewhat diffuse and lacks sharp boundaries.

In terms of color, the central bulge displays a yellowish hue, which likely indicates an older stellar population. The outer regions appear slightly bluer, suggestive of ongoing star formation in these areas. There might be a slight disturbance present, although it does not look like it is in the middle of a large merging event. Overall, it is an isolated galaxy.
