The galaxy presents as a relatively smooth, elongated structure. It exhibits a clear central bulge, which appears a yellow-orange hue, possibly indicating an older stellar population.  A disk component is faintly visible, extending beyond the bulge. The disk is relatively featureless, with no obvious spiral arm structure discernable at this resolution, potentially indicative of a more lenticular morphology.  The disk shows some blue light, possibly from younger stars and on-going star formation, though this is not pronounced. The overall structure appears largely undisturbed, showing little evidence of any major interactions or mergers, though there is a hint of slight distortion on one side. The elliptical shape is moderately elongated.
