This galaxy presents a somewhat elliptical morphology. The light distribution is generally smooth and centrally concentrated, but it's difficult to discern any distinct features. The color gradient transitions smoothly from a slightly yellowish-white core region towards fainter, bluer outskirts, suggesting a possible radial change in stellar population or dust content. The overall structure shows a suggestion of disruption or interaction, possibly a minor tidal disturbance. While no obvious spiral arms are visible, the light distribution isn't perfectly uniform, indicating some underlying structure. The galaxy is relatively compact, with no apparent extended halo or tidal features dominating the immediate surroundings.
