The galaxy presents a generally smooth, elliptical morphology, displaying a relatively high degree of central concentration. Its shape appears to be somewhat elongated, trending towards a cigar-like appearance. The light distribution is dominated by a central bulge, exhibiting a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer regions extend from the core, indicating the presence of younger stellar populations and possibly ongoing star formation, though at a low rate. There is no evidence of spiral arm structures or a prominent disk. The galaxy's overall structure appears undisturbed, with no obvious signs of recent major mergers or tidal interactions, although some minor irregularities in the outer regions cannot be ruled out.
