The galaxy presents as a concentrated, centrally luminous object with a generally smooth morphology. There is a subtle decrease in luminosity from the core to the outer regions. Based on the color profile, the central region appears to be composed of an older stellar population, indicative of a high concentration of evolved stars, suggesting a potential elliptical classification. There is a hint of a very subtle disk, but it appears to be a spiral galaxy that has had much of it's star formation cease.

Based on the visual inspection, there is no significant evidence of tidal disturbances, major ongoing mergers, or prominent star formation regions. This is supported by the lack of intense blue color, which would signify rapid star formation. While not perfectly spherical, it deviates only subtly from a circular profile, presenting a general lack of elongation.
