This galaxy exhibits an elliptical morphology, with a smooth, centrally concentrated light profile. The color gradient suggests an older stellar population, with the core appearing more yellowish and the outer regions showing hints of bluer hues. The galaxy is moderately elongated, displaying a cigar-like shape. There's no obvious presence of distinct spiral arms or a prominent dust lane. The overall structure suggests that the galaxy is not currently undergoing any major merging events, although subtle disturbances may be present. The light distribution is generally smooth and symmetrical, indicating a lack of significant ongoing star formation. The galaxy's size, combined with its color profile, indicates that the galaxy is a relatively large and massive system.
