The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth with a concentrated central bulge that dominates its overall luminosity. The bulge exhibits a yellowish hue, possibly indicative of an older stellar population. Moving outwards from the center, a faint disk is barely discernible, marked by a subtle blueish tint. There are no prominent spiral arms or distinct dust lanes visible within this disk. The galaxy seems to be undergoing little to no significant star formation, and appears undisturbed, with no readily apparent signs of recent merger activity or tidal distortions.
