The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology with no prominent spiral arms or obvious disk structure. The light distribution suggests a centrally concentrated bulge, with the overall shape appearing roughly rounded, although possibly slightly elongated. There may be a faint, extended halo surrounding the central region. There does not appear to be any evidence of a major merger event, although there may be some subtle internal disturbances or asymmetries. The color profile indicates an older stellar population, with a yellow/red hue dominant in the central region. Star formation appears to be minimal within the galaxy, however, some small star forming regions may be present.
