The galaxy presents as a relatively smooth, cigar-shaped structure. It exhibits a concentrated, bright central bulge, surrounded by a fainter, elongated disk. The color profile suggests a dominance of older stellar populations, with a yellow-red hue prevalent throughout the galaxy, particularly within the bulge. There's limited evidence of distinct spiral arms or prominent dust lanes. The galaxy displays a generally undisturbed morphology, with no obvious signs of major mergers or significant tidal interactions. Subtle irregularities or minor disturbances may be present but are not immediately apparent at this resolution.
