The galaxy presents a generally smooth, elliptical morphology. It appears concentrated, with a bright central bulge that transitions into a slightly fainter extended halo. The color profile indicates a relatively older stellar population, with a redder hue dominating the central regions, transitioning to slightly bluer shades in the outer halo. There appears to be little evidence of active star formation regions within the galaxy, nor is there any obvious sign of spiral arm structure or a prominent dust lane. There appears to be slight asymmetry within the outer halo which could indicate some minor gravitational interaction in the past. Overall, the galaxy appears to be a fairly evolved system, potentially nearing the end of its star-forming period.
