The galaxy presents as a somewhat smooth, elongated structure. Its shape is reminiscent of a flattened spheroid, appearing cigar-shaped. The color gradient transitions from a brighter, more yellowish-white central bulge region to a dimmer, redder outer disk. Evidence of any prominent spiral arms is lacking; the overall light distribution appears relatively uniform. There are hints of slight disturbances. The absence of distinct features suggests that it may be a relatively evolved system. Star formation activity appears low. There is some dust content. The galaxy is likely to be a large, massive system.