This galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile is dominated by yellowish hues, suggesting a stellar population that is primarily composed of older, redder stars. There is no evidence of significant dust lanes, spiral arms, or active star formation regions visible in this image. The galaxy appears to be fairly isolated, with no obvious signs of major tidal distortions or ongoing merger activity. It is generally round in appearance, with only a slight elongation. There are no features indicative of significant disruption or morphological peculiarities.
