The galaxy presents an overall smooth morphology. It appears elongated with a cigar-shaped structure. A bright central bulge is visible, surrounded by a fainter extended halo or disk. There is no visual evidence of strong spiral arm structure or significant dust lanes. The galaxy appears to be relatively undisturbed, without clear signs of ongoing major merging activity. Its color profile suggests a somewhat evolved stellar population, with light emitted across the g, r and z bands.
