The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. There appears to be a faint disk surrounding the bulge. The color profile suggests a mix of stellar populations. The central bulge exhibits a bluer hue, potentially indicating a younger, hotter stellar population or active star formation. Fainter, redder material surrounds the brighter core, suggesting an older stellar population may be present within the disk. There are subtle hints of asymmetrical features, possibly indicating minor gravitational interactions or disturbances. There is some slight evidence of tidal tails extending from the central bulge. The galaxy does not appear to be a pure elliptical, and exhibits slight irregularities and possible disturbances of its form.
