The galaxy presents a flattened, elliptical morphology with a relatively smooth light distribution. The galaxy exhibits a bright, concentrated central bulge that graduates into a less defined disk. The major axis is noticeably longer than the minor axis. The color profile appears to be somewhat redder in the central regions, suggesting an older stellar population, while the outer regions appear slightly bluer, potentially indicating ongoing or recent star formation. There's no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of a major merger or tidal interactions.
