The galaxy presents as a single, largely featureless object. It exhibits a centrally concentrated luminosity profile with no discernible spiral arms, bar structure, or distinct nucleus visible at this resolution. The galaxy appears roughly circular in shape, showing high degree of symmetry. The color profile is indicative of a evolved stellar population, trending towards redder hues, though there is evidence of some bluer regions within the galaxy. There is no clear evidence of any ongoing major merging events or tidal disturbances in the immediate vicinity of the galaxy.
