The galaxy presents a generally smooth and rounded morphology, exhibiting a centrally concentrated luminosity profile. The light is relatively homogenous, with no prominent spiral arm structures or bar features discernable. The galaxy appears slightly elliptical. The color index, inferred from the RGB values, suggests a moderately red population, potentially indicating an older stellar population and/or significant dust content. There is no visual evidence of active galactic nuclei activity, such as jets or a bright point source at the center. There is a hint of a possible faint extension or tidal feature at the edges. The galaxy does not seem to be undergoing any major merging event with another galaxy. The apparent size suggests that it is a medium sized galaxy.
