The galaxy presents as a slightly elongated, lenticular-like structure. The light distribution appears smooth and centrally concentrated, suggesting an older stellar population. There may be a slight hint of a disk component. The galaxy displays a color gradient, with the core region exhibiting a yellower, more reddish hue, likely indicative of older stars or dust obscuration, while the outer regions appear somewhat bluer, possibly suggesting recent star formation. There are no prominent spiral arms or other well-defined features discernible at this resolution, which indicates that there has not been a recent major merger. The absence of significant morphological disturbances suggests relative quiescence in its recent dynamical history. It could be characterized as an intermediate-mass galaxy based on its approximate size and luminosity.
