The galaxy presents an elliptical morphology, appearing cigar-shaped in projection. There is a smooth, centrally concentrated light distribution with a notable color gradient. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions towards a slightly redder tone.  There is no readily apparent evidence of spiral arm structure. The overall form suggests a galaxy undergoing relatively little current star formation activity. There may be some minor tidal disturbance on the edge of the galaxy, but this is not definitive and it's likely the system is not undergoing a major merger.
