The galaxy presents as a relatively compact object with a smooth, centrally concentrated light distribution. It exhibits an overall elliptical morphology, appearing mostly rounded, with only a slight deviation towards a cigar shape. The galaxy's color profile suggests a more evolved stellar population, with a noticeable concentration of light in the redder wavelengths towards the central region, likely indicating older, cooler stars. There's some evidence of slightly bluer light, suggesting some star formation is occurring, but overall, the galaxy doesn't appear to be undergoing intense starburst activity. No significant signs of spiral arms, bars, or tidal features are detected, indicating the galaxy is unlikely to be undergoing major mergers or strong gravitational interactions. Small disturbance is possibly observed. The estimated mass of the galaxy is likely to be between 10^9 and 10^9.5 solar masses.
