The galaxy presents an overall smooth morphology, suggesting a relatively evolved system. It exhibits a slightly elongated, cigar-shaped structure. The light distribution appears concentrated towards the center, characteristic of a bulge, with a gradual fall-off in intensity towards the outer regions.

There is evidence of possible minor disturbances. Although the galaxy generally appears smooth, there are some subtle indications of non-uniformity in the light distribution, potentially indicating past or ongoing interactions. Some components may be in the process of merging.

The galaxy displays a redder color, concentrated in the core region, possibly indicating an older stellar population dominated by evolved stars. Overall, the galaxy appears to be relatively massive and has a moderate rate of star formation.
