This galaxy presents as a relatively bright, elongated structure. Its light is concentrated towards the center, suggesting a significant bulge component. There appears to be a disk structure, although it is not sharply defined. The color profile indicates a population of older stars dominating the galactic structure. This galaxy does not have an obvious spiral arm structure. There is a slight irregularity or distortion visible in the outer regions of the disk, possibly indicating past interactions or mergers. The overall morphology suggests an elliptical leaning towards lenticular galaxy with some disturbances present.
