The galaxy presents an overall smooth morphology with a noticeable lack of spiral arm structure. Its shape appears to be somewhat elongated, exhibiting an elliptical form rather than a perfect sphere. The central region displays a significantly higher surface brightness, suggesting a concentrated nucleus likely comprised of older stellar populations. The color profile is dominated by redder hues, indicating a relative paucity of young, massive stars and ongoing star formation activity, which is consistent with the smooth, featureless morphology. The galaxy exhibits a faint, diffuse halo extending beyond its core, gradually fading into the background. There is no readily apparent sign of any major mergers or tidal disturbances.
