The galaxy presents as a moderately faint, diffuse object, exhibiting a roughly elliptical morphology. There's a subtly brighter, somewhat compact core region with a pale blue-white hue, implying the presence of a younger stellar population and perhaps ongoing or recent star formation, though at a relatively low rate. The outer regions of the galaxy appear fainter and more irregular, suggesting a less concentrated distribution of stars. There is a slight hint of disturbed features. There may have been a minor interaction or merger event in the past, or simply some internal dynamical processes at play. Overall, the galaxy appears to be relatively small.
