The galaxy exhibits a dominant, smooth spheroid component indicative of an elliptical or lenticular morphology. The light distribution suggests a centrally concentrated profile with a gradual decline in intensity towards the outer regions. There's a subtle elongation to the galaxy's shape, though it appears largely round, with no clear signs of spiral arms or prominent disk features. The primary color is yellowish-orange, consistent with an older stellar population dominated by redder stars. No strong dust lanes or active star-forming regions are readily apparent in the image. The overall appearance is suggestive of a relatively passive galaxy with little ongoing star formation. A slight disturbance of the light surrounding the galaxy may indicate a past or ongoing minor merger, but the primary structure remains largely undisturbed.
