The galaxy appears as a concentrated, relatively smooth elliptical. The core region exhibits a bright, diffuse glow, with the highest intensity. A faint, extended halo of light surrounds the central region, gradually fading into the background. There may be some faint indication of spiral arm structure, or possibly tidal tails, but these are unclear. The color gradient suggests an aging stellar population, with a central bulge dominated by older, redder stars. Star formation is likely minimal in the main body. The galaxy appears to be relatively isolated, not displaying obvious signs of a major merger. Faint distortions suggest potential minor interactions, or perhaps internal dynamics affecting the morphology on a smaller scale. Overall, the galaxy presents a relatively regular, evolved form.
