The galaxy appears as a cigar-shaped or elliptical object. It exhibits a relatively smooth morphology, with a noticeable central bulge. The galaxy's light is concentrated in the central region, with a gradual decrease in brightness towards the outer edges.  A slight color gradient is observed, with a bluer hue in the central region, potentially indicating ongoing star formation, and a shift towards redder colors in the outer regions, suggesting an older stellar population.  There is no indication of significant tidal disturbances or major mergers. The galaxy is a relatively compact structure. There seems to be a small population of star formation, but the overall star formation rate appears to be low. It is likely a galaxy with a significant amount of its mass already formed.
