The galaxy presents as a relatively smooth, elliptical-like structure. There is an apparent central bulge exhibiting a concentrated luminosity gradient. Proceeding outwards from the core, the light gradually decreases, appearing as a diffuse halo. The shape is elongated, indicating a possible elliptical morphology with notable ellipticity. The color profile suggests a population of older stars, exhibiting a redder hue. A possible tidal interaction is occurring, and there are minor disturbances visible in the galaxy structure. There appears to be a possible merger occuring on the edges of the galaxy. Star formation activity appears to be low or negligible, indicated by the lack of significant blue color. The galaxy is approximately 7 kiloparsecs in radius.