The galaxy presents as a relatively smooth, centrally concentrated object. There is an elliptical appearance with a slightly elongated shape, exhibiting a minor deviation from a perfect circular form. The central region displays a higher luminosity, suggesting the presence of a prominent galactic nucleus. A subtle gradient in color is observed from the core outwards with a shift towards redder hues, suggesting a population of older stars in the outer regions. While subtle, faint disk-like features are weakly discernable. Overall, the galaxy appears to be undergoing moderate star formation. Evidence suggests there is no ongoing major merging events, although minor disturbances cannot be ruled out. The galaxy appears to be of moderate size.