The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile with no distinct spiral arms or bar structure visible. The central region displays a concentration of yellow-white light, suggesting an older stellar population. A slight elongation is observed, indicating it's not perfectly spherical, but rather somewhere between round and cigar-shaped. The outer regions of the galaxy fade gradually into the background sky, lacking any sharp boundaries. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances, although a minor interaction cannot be completely ruled out based on the slight irregularity of the light distribution. The observed color gradient suggests some level of on-going star formation is likely, though at a relatively low rate, with a bias towards more red-shifted wavelengths.
