The galaxy presents as a relatively compact and moderately bright object. Its overall morphology appears to be largely smooth and featureless, lacking any prominent spiral arms or a distinct bar structure. The light distribution suggests a spheroidal shape, although there is a slight elongation visible. There is a concentration of light towards the central region, indicative of a galactic nucleus. The galaxy exhibits a color gradient, transitioning from a bluer hue at the outskirts to a redder hue towards the center. There is no evidence of significant ongoing major merging activity or tidal disturbances in its immediate vicinity, however minor disturbances cannot be ruled out. The colors displayed indicate a population of older stars. The galaxy’s apparent size is small, suggesting it is either intrinsically small or at a significant distance.
