The galaxy presents as a somewhat elongated, cigar-shaped structure. There is a central bulge which appears to be a dominant feature, characterized by a yellowish-orange hue indicative of an older stellar population. Extending outwards from the bulge, a disk is faintly visible, showing hints of bluer regions, particularly at the edges, possibly indicating areas of more recent or ongoing star formation, although overall the blue fraction seems low. There are no prominent spiral arm structures immediately discernible, and the disk appears relatively smooth. The galaxy exhibits no obvious signs of tidal distortions or major mergers. The overall color profile leans towards the redder end of the spectrum, suggesting a galaxy with a significant population of evolved stars and a suppressed star formation rate. The galaxy appears to be a relatively massive system.
