The galaxy presents a generally smooth morphology, with a central concentration of light that appears nearly spheroidal. The color profile suggests a population of older stars, particularly within the central bulge which exhibits a yellowish hue. Fainter, bluish extensions are present, possibly indicating areas of more recent, though subdued, star formation within what may be a faint disk. There is no clear evidence of strong spiral arm structure or a distinct bar feature. A slight asymmetry could be suggestive of minor tidal interaction, or could be simply internal irregularities. No strong signs of a major merger are apparent.
