The galaxy presents an overall elongated morphology, appearing cigar-shaped in its major axis. The central region exhibits a relatively smooth light distribution, suggesting a high concentration of stars within a spheroidal component, possibly a bulge. There are some disturbances in the form of clumps of light, possibly star forming regions. The galaxy shows a color gradient, with the central region appearing yellower, and the outer regions exhibiting bluer tones. This color variation may indicate differences in stellar populations, with older stars dominating the central bulge and younger, hotter stars residing in the more extended regions. The galaxy is quite faint, requiring careful examination to discern its structural details. No prominent spiral arms are visible, and the overall structure appears relatively featureless beyond the central concentration. There is also a minor amount of disruption visible.
