The galaxy presents as a well-defined elliptical structure. Its shape is elongated, with the major axis being significantly longer than the minor axis, exhibiting an axis ratio of approximately 0.5. The overall color appears relatively blue-white, suggesting the presence of a moderately young stellar population. The light distribution is centrally concentrated, with a bright core that fades smoothly outwards. There is little evidence of spiral arms or distinct features typically associated with spiral galaxies. The galaxy appears relatively undisturbed, showing no strong signs of recent mergers or tidal interactions. Its size is relatively small compared to other galaxies, but the light distribution is still clear enough to determine morphological features.
