The galaxy presents a morphology that appears largely smooth. There is some indication of substructure; the galaxy is elongated and slightly irregular rather than perfectly spherical, suggesting a degree of dynamical disturbance within the system, possibly the early stages of interaction with another galaxy.

The galaxy has a noticeable color gradient, with a central, condensed region displaying a yellowish-orange hue, and more diffuse outer regions having a slightly bluer tint. This color difference could be attributed to varying stellar populations within the galaxy, with older, redder stars dominating the core and younger, bluer stars residing in the outer regions. The estimated size is 6.5 kiloparsecs.

While the majority of the light is concentrated centrally, there is no clearly defined spiral arm structure visible. The lack of prominent spiral arms coupled with the smoothness of the overall light distribution would indicate that the galaxy is likely an elliptical or lenticular type. Overall this is a typical galaxy undergoing star formation.
