The galaxy presents as a luminous, elongated structure with a relatively smooth appearance. Its color profile indicates a yellow-orange hue, concentrated primarily toward the central region, suggesting a substantial population of older stars. The outer regions exhibit a bluer tint, possibly indicating the presence of younger stellar populations and some ongoing star formation.

The galaxy's morphology seems elliptical with an apparent lack of distinct spiral arm structures or a prominent disk, viewed at a steep angle. The light distribution decreases steadily from the center towards the edges, contributing to the overall smooth appearance. There's no apparent evidence of major mergers or tidal disturbances within the immediate vicinity of the galaxy.

