The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution is dominated by yellowish-orange hues, suggestive of an older stellar population and a lower rate of ongoing star formation. It does not appear to have strong spiral arm structures or significant dust lanes. The morphology seems to be more spheroidal in nature with some elongation, appearing somewhat cigar-shaped rather than perfectly circular. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances based on the image. There is a slight hint of bluer emission at the edge of the structure, which could indicate more recent star formation occurring in that region, but the dominant color suggests an evolved population of stars and lower star forming activity. Overall, the galaxy appears as an early-type galaxy, likely an elliptical or lenticular galaxy, at an appreciable distance.
