The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a higher surface brightness, appearing more concentrated and yellowish in color. Moving outwards from the core, the light gradually fades and the color transitions toward a bluish hue. There is no prominent evidence of spiral arms or a distinct disk structure. The overall shape is somewhat rounded, with only a slight elongation. No obvious signs of recent or ongoing major merger events are apparent, although subtle irregularities in the outer regions could indicate minor disturbances or tidal interactions. The object appears fairly isolated in this particular field of view. The galaxy is estimated to be fairly massive, and exhibits a moderate star formation rate.
