The galaxy presents as a relatively bright, centrally concentrated system with an overall smooth appearance. The core region exhibits high luminosity, exhibiting an elliptical morphology. The light distribution fades gradually outward from the core, suggesting a high degree of radial symmetry. There appears to be faint, diffuse structure extending along the major axis, but no distinct spiral arms or bar are discernible. The galaxy’s color is generally consistent with an older stellar population, with a slight reddish hue particularly pronounced towards the core. No significant dust lanes or regions of active star formation are immediately apparent, and the galaxy appears to be relatively isolated. The galaxy does not seem to be undergoing any major merging events. Overall, the galaxy presents characteristics consistent with an elliptical galaxy type.
