The galaxy presents as a relatively compact object. It exhibits a centrally concentrated luminosity profile, appearing smooth with a lack of distinct spiral arm features or a prominent bulge. The overall shape appears roughly elliptical, though not perfectly circular. There is a suggestion of some internal structure or faint extension visible in the galaxy’s periphery, hinting at possible interactions or minor disturbances. The colour is biased towards blue, indicating the presence of some younger, hotter stars, although redder regions are present. There is no strong evidence of major merging activity, such as tidal tails or distorted morphology. The galaxy appears to be relatively isolated, with no immediately obvious companion galaxies nearby within the field of view.
