The galaxy appears as a moderately luminous, elongated object. Its shape is suggestive of an elliptical galaxy, although some characteristics suggest a possible disk component. The galaxy's light is concentrated toward the center, indicating a central bulge. The galaxy appears to be generally smooth in texture, without obvious spiral arm features, major disturbances, or significant signs of recent merger activity. The color profile indicates a population of relatively older stars with modest star formation. The galaxy is likely to be of intermediate mass. The apparent color suggests it is at intermediate redshift. Overall, the galaxy presents a moderately luminous system with characteristics of both an elliptical galaxy and a spiral galaxy. Further spectroscopic data would be useful for confirming its type and for determining its velocity with greater accuracy.
