The galaxy presents as a fairly compact, elliptical-like structure with a smooth, concentrated central bulge. Its color profile leans towards the redder end of the spectrum, indicating an older stellar population with a lower rate of ongoing star formation. There appears to be a slight asymmetry to its shape, possibly indicative of a minor gravitational interaction or disturbance. I see little evidence of spiral arms or a prominent disk component, and the galaxy's overall morphology suggests it is a relatively undisturbed system, not currently undergoing a major merger.
