The galaxy presents as an elongated, cigar-shaped structure, with a distinct central bulge. The core appears to be a bright yellowish hue, indicative of an older stellar population and potentially high dust concentration in the nucleus. Fainter, diffuse bluish light extends from the bulge along the major axis, suggesting the presence of younger, hotter stars in these regions. This implies ongoing, albeit subdued, star formation is likely occurring within the galaxy's disk. The overall structure is relatively smooth, without any obvious signs of recent major mergers or tidal disruptions. The light distribution fades gradually toward the edges, suggesting a relatively undisturbed disk. It seems to be an elliptical galaxy.
