The galaxy appears to be an elliptical system, exhibiting a generally smooth morphology. The light distribution is concentrated towards the center, with a decrease in brightness radiating outwards, indicating a relatively high degree of central mass concentration. The shape is somewhat rounded, though not perfectly circular. The color is primarily yellowish-orange, suggesting a population of older stars and a low rate of ongoing star formation. There are some subtle indications of disturbances in the galaxy's shape, potentially hinting at past or ongoing interactions with another galaxy. Possible minor disturbance or tidal feature could be present. The system has an extended halo but no clearly visible spiral arms or prominent dust lanes. Overall, the galaxy seems to be a massive, evolved system with only a low-level of recent star formation.
