The galaxy presents a generally smooth, elliptical morphology. The object appears to be moderately massive, exhibiting a concentrated central bulge that transitions into a less defined, extended halo. The color profile suggests an evolved stellar population, with a yellow-red hue indicating a preponderance of older stars. The isophotes are relatively regular, without prominent spiral arm structures or significant dust lane features. There may be a subtle tidal disturbance or minor interaction apparent in the outskirts of the halo, but this is relatively minor. The overall structure appears to be fairly well-relaxed, characteristic of a galaxy with minimal ongoing star formation.
