The galaxy appears as a moderately bright, elliptical-shaped object. The light distribution is relatively smooth, with a higher concentration towards the center, suggesting a prominent bulge. The galaxy's color gradient indicates a population of older stars contributing to the redder hues, particularly in the central regions. There is no apparent dust lane or spiral arm structure visible in this image, further supporting an elliptical classification. The galaxy seems relatively isolated with no close companions. There is minimal indication of ongoing star formation. The galaxy is slightly elongated, appearing cigar-shaped rather than perfectly circular. There appears to be no strong tidal disturbance or signs of an active merger event.
