The galaxy presents an elongated, disk-like structure viewed at an angle, appearing somewhat cigar-shaped. The central region exhibits a bright, concentrated luminosity indicative of a bulge. The color distribution suggests a range of stellar populations, with the central bulge appearing more yellow, likely indicating older stars. Fainter, bluish or greenish hues are observed in the outer disk, possibly denoting areas of ongoing star formation. The disk appears relatively smooth, without prominent spiral arm structures visible at this resolution. There is no evidence of significant tidal disturbances or major mergers in the immediate vicinity of the galaxy. The overall morphology suggests a relatively evolved galaxy with a moderate level of star formation.
