The galaxy presents a generally smooth appearance, with a dominant, luminous central bulge. There is evidence of a disk component surrounding this bulge. This disk structure is not particularly well-defined, suggesting the galaxy is relatively early-type and exhibits a small amount of disk structure. The galaxy appears somewhat flattened. The color profile suggests an older stellar population, particularly within the bulge. There are some features within the disk that imply some ongoing star formation is occurring. The galaxy does not appear to be undergoing a major merger or strong tidal interaction with another galaxy, though the slight distortions might suggest minor interactions are ongoing.