The galaxy exhibits a relatively smooth, elliptical morphology. Its color is generally yellow-orange, suggesting a dominant population of older stars with lower rates of star formation. There appears to be a concentrated central region, likely a bulge, surrounded by a more diffuse halo. No obvious spiral arms or dust lanes are visible. The overall shape appears approximately round, with only minor deviations from a perfect circular form. There is no strong evidence of ongoing or recent major merging events, or significant tidal disturbances within the immediate vicinity of the galaxy.
