The galaxy presents a generally elliptical morphology, exhibiting a smooth, featureless structure with no immediately apparent spiral arms or bar. Its color profile suggests an older stellar population, appearing relatively redder than galaxies actively undergoing significant star formation. The galaxy's light is centrally concentrated, indicative of a prominent bulge. There is a subtle decrease in surface brightness moving from the core towards the outer edges. The isophotes exhibit a slight ellipticity, deviating marginally from a perfectly circular shape. Overall, the galaxy appears consistent with an early-type galaxy, likely an elliptical or lenticular (S0) galaxy, exhibiting little to no recent or ongoing star formation within the visible spectrum.
