The galaxy presents an elliptical or lenticular morphology, characterized by a smooth, diffuse light distribution. The primary component exhibits a bright, relatively blue hue, possibly indicating a region of active star formation or the presence of a significant population of hot, young stars. A secondary, more subdued component is observed adjacent to the primary, displaying a yellowish color, which could be attributed to an older stellar population. The galaxy exhibits a moderate degree of roundness. There appears to be a suggestion of tidal interactions. The approximate effective radius of the galaxy is several kiloparsecs. The absolute magnitude of the galaxy is quite high, suggesting a high luminosity.
