The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. The color gradient suggests a population of older stars dominating the galaxy's light output, with a likely absence of significant ongoing star formation. There is a slight elongation, giving it a cigar-like shape, but no obvious features indicating spiral arms or a bar structure. No signs of tidal interactions or significant disturbances are apparent in the image, suggesting it is likely a relatively isolated system. The object exhibits a color profile that is redder towards the center, which is consistent with the presence of an older stellar population and dust accumulation in the core.
