The galaxy presents as an elongated, somewhat cigar-shaped structure. Its central region exhibits a brighter, more concentrated luminosity, possibly indicating a dense galactic nucleus or bulge. Moving outward from the center, the light diffuses, fading toward the edges of the galaxy.

The color profile appears relatively uniform, with a suggestion of bluer hues, potentially indicative of ongoing star formation or a younger stellar population. There are no immediately obvious indications of prominent spiral arms or significant dust lanes. The overall smoothness of the light distribution hints at an elliptical morphology, but some subtle irregularities suggest the possibility of past or ongoing minor interactions. There are no prominent tidal tails or other signs of major mergers.
