The galaxy presents as an elongated, cigar-shaped structure. Its overall light distribution appears relatively smooth, with a bright, concentrated central bulge. Some asymmetry is present, with a subtle extension visible at one end, suggesting a possible tidal feature or minor disturbance. Color gradients indicate a redder core, potentially indicative of an older stellar population, shifting towards bluer hues in the outer regions, possibly indicating younger stars. This galaxy is approximately 3.9 kpc in radius, and the light observed suggests the presence of ongoing star formation. There is no indication of major recent merger activity or significant disturbances in the galaxy's overall structure.