The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions are observed surrounding the bulge, potentially indicating areas of ongoing star formation within the galaxy's disk. There appears to be some degree of disk structure, though it is not sharply defined. No strong indications of spiral arms or a bar are discernible from the image. The overall morphology leans towards a smooth appearance, yet some features or disturbances are likely present, though not immediately apparent at this resolution. It doesn't appear to be undergoing a major merger, however there is a possibility for minor disturbances or interactions.
