The galaxy presents as a relatively compact object with a discernible disk-like structure. The overall morphology appears to be neither purely elliptical nor a grand design spiral; instead, it exhibits characteristics suggestive of an intermediate type. The light distribution is centrally concentrated, with a smooth, gradual decline in intensity outward from the core.

While there's no strongly defined spiral arm structure, faint hints of features or irregularities are visible in the disk. The color profile indicates a slightly redder hue, potentially indicating an older stellar population and/or a higher dust content. There isn't strong evidence of recent star formation, such as bright blue regions or prominent HII regions. Signs of any major interactions or mergers are not readily apparent from the galaxy's overall appearance; it seems to be relatively undisturbed.
