The galaxy presents as a generally smooth, luminous object with a somewhat elliptical morphology. There is a bright central bulge that appears roughly spherical, surrounded by a less concentrated, more diffuse halo. The color profile suggests the presence of both older stellar populations within the bulge, exhibiting a yellow-orange hue, and possibly some regions of ongoing star formation in the outer disk, indicated by a faint bluish tint. There is a subtle asymmetry in the halo, possibly indicating a minor gravitational interaction or disturbance in the recent past. The galaxy does not present any strong visual signs of a major ongoing merger, nor does it appear to be a classic spiral structure. It is likely an intermediate-mass galaxy with moderate star formation.
